BackForwardInstrument:  SOT 

Instrument details
Acronym SOT
Full name Solar Optical Telescope
Purpose To obtain continuous high-resolution magnetic field imagery of the sun's surface
Short description Photospheric and chromospheric imaging and spectropolarimetry in the 480-650 nm VIS range. The band includes several lines of Iron whose Doppler analysis enables inference of the vectorial magnetic field at the photosphere
Background Part of a package of instruments for solar observation
Scanning Technique Sun pointing from a dawn-dusk LEO
Resolution 175 km at Sun surface
Coverage / Cycle Full solar disk at 10 s intervals
Mass Power Data Rate 300 kbps

 

Providing Agency JAXA
Instrument Maturity Flown on an R&D satellite
Utilization Period: 2006-12-22 to 2016-02-25
Last update: 2017-05-19
Detailed characteristics
Satellites this instrument is flying on

Note: a red tag indicates satellites no longer operational, a green tag indicates operational satellites, a blue tag indicates future satellites

Instrument classification
  • Solar and space environment monitors
  • Solar activity monitor
Mission objectives
Primary mission objectives
  • Solar electric field
  • Solar magnetic field
  • Solar velocity fields
Opportunity objectives
  • Solar VIS flux spectrum
  • Solar VIS image
Show allShow fewer
Tentative Evaluation of Measurements

The following list indicates which measurements can typically be retrieved from this category of instrument. To see a full Gap Analysis by Variable, click on the respective variable.

Note: table can be sorted by clicking on the column headers
VariableRelevance for measuring this variableOperational limitationsExplanation
Solar VIS flux spectrum1 - primaryNo specific limitation.High spectral resolution, moderate dynamic range, polarimetry and Doppler shift exploited
Solar VIS image1 - primaryNo specific limitation.Spectrometry with high spatial resolution, polarimetry and Doppler shift exploited
Solar magnetic field1 - primaryNo specific limitation.Spectrometry with high spatial resolution, polarimetry and Doppler shift exploited
Solar electric field1 - primaryNo specific limitation.Spectrometry with high spatial resolution, polarimetry and Doppler shift exploited
Solar velocity fields1 - primaryNo specific limitation.Spectrometry with high spatial resolution, polarimetry and Doppler shift exploited